First detection and characterization of the gas feeding star formation around nearby galaxies observed with MUSE
Using the publicly available cosmological fields of MUSE, we plan to detect the gas that feeds star formation in nearby galaxies. It would be the first time this gas is detected in Ha. The main advantage of using Ha with respect to Lya (used at high redshift) is the possibility of measuring metallicity and, thus, to be able to distinguish between
Jorge Francisco
Sánchez Almeida
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